Source: Celestial Mechanics and Dynamical Astronomy. Unidade: IAG
Subjects: CAOS (SISTEMAS DINÂMICOS), PLANETAS, PULSARES, SISTEMA SOLAR
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CALLEGARI JÚNIOR, Nelson e FERRAZ-MELLO, Sylvio e MICHTCHENKO, Tatiana Alexandrovna. Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12. Celestial Mechanics and Dynamical Astronomy, v. 94, n. 4, p. 381-397, 2006Tradução . . Acesso em: 16 nov. 2024.APA
Callegari Júnior, N., Ferraz-Mello, S., & Michtchenko, T. A. (2006). Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12. Celestial Mechanics and Dynamical Astronomy, 94( 4), 381-397.NLM
Callegari Júnior N, Ferraz-Mello S, Michtchenko TA. Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12. Celestial Mechanics and Dynamical Astronomy. 2006 ; 94( 4): 381-397.[citado 2024 nov. 16 ]Vancouver
Callegari Júnior N, Ferraz-Mello S, Michtchenko TA. Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12. Celestial Mechanics and Dynamical Astronomy. 2006 ; 94( 4): 381-397.[citado 2024 nov. 16 ]
